The galaxy presents an overall smooth appearance, with a noticeable elongation along a defined axis. While a central bulge is not clearly distinct, there is a concentration of light towards the center, which is also a slightly redder hue compared to the outer regions. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy appears relatively undisturbed, without any major signs of tidal interactions or ongoing mergers. A very minor disturbance cannot be ruled out based on the irregularities in the shape. There is no significant central bar. Based on the color profile, the object likely contains a moderately aging stellar population and a low rate of ongoing star formation. The galaxy appears to be on the smaller side compared to average galaxies.
