The galaxy presents as a moderately luminous, elongated object. Its morphology appears to be somewhere between a lenticular and an elliptical galaxy, as it exhibits a generally smooth profile with a hint of disk-like structure, although no spiral arms are clearly visible. The color profile of the galaxy shows a bulge with a central concentration of light, with a yellow-white hue, implying a relatively older stellar population dominating the core, with a potential of some dust extinction present around the central regions. The outer regions display a subtle color shift towards redder hues. There is no strong evidence of active star formation regions. It does not appear to be undergoing any major merger events or significant tidal disturbances based on its overall morphology. There are indications that there may be very minor tidal disturbances, but not in the form of a merger. The shape is cigar-like in shape, with some in-between characteristics.