The galaxy presents as a somewhat elongated, lenticular-like structure. It exhibits a centrally concentrated brightness profile, suggesting the presence of a bulge. The overall color is yellowish-white, with hints of blue in what may be a very faint, loosely defined disk component. There is minimal evidence of spiral arm structure or prominent dust lanes within the galaxy. The overall texture appears smooth, implying a relatively old stellar population dominating the light output. There are hints of minor irregularities or disturbances in the galaxy's morphology, possibly indicative of a past or ongoing minor interaction.
