The galaxy presents as a faint, diffuse object of moderate angular size. Its morphology appears disturbed, with a subtle elongation and asymmetries in the distribution of light. The overall color profile is skewed towards the redder end of the spectrum, with a weak signal in the green channel. There is no clear evidence of a spiral structure or prominent disk. Instead, the light appears to be distributed in a more irregular fashion, possibly indicative of a recent or ongoing interaction with another galaxy. A slight deviation in the galaxy's overall form is visible, possibly due to the presence of a minor tidal disturbance. The galaxy's core region seems more concentrated, but lacks the distinct appearance of a well-defined nucleus. There are no readily visible, strong star-forming regions within the galaxy, suggesting a relatively quiescent state. The general appearance is consistent with an elliptical galaxy undergoing some minor interaction, or potentially a very faint, disrupted spiral.
