The galaxy presents as a system with a central, bright bulge dominating the light profile. This central region exhibits a yellowish hue, possibly indicative of an older stellar population. Extending outwards from this bulge is a fainter, less defined disk. The disk shows hints of bluer colors which may indicate areas of more active star formation. There appears to be a minor tidal disturbance or faint arm-like structure extending from the central bulge, with asymmetric distribution in relation to the bulge itself. This structure may indicate an interaction with a smaller galaxy. The galaxy exhibits an intermediate shape, between round and elongated, with a mild cigar shape morphology. The overall structure seems to be reasonably undisturbed, with no strong signs of ongoing major merger activity.
