The galaxy presents as a somewhat elongated, cigar-shaped structure. The central region exhibits a bright, smooth appearance, with a concentrated light profile. The color suggests an older stellar population, possibly dominated by redder stars, with hints of younger, bluer populations in the outer regions. There are disturbances observed, but they are not significant. Based on the slight disk-like appearance, I believe it may be a relatively smooth spiral galaxy with tightly wound arms or a lenticular galaxy viewed at an angle. I believe it is undergoing a minor merger due to slight asymmetry. Star formation appears to be relatively low.
